Poster + Paper
26 August 2022 SAMpy: a Fourier-plane pipeline for JWST/NIRISS aperture masking interferometry (and more!)
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Conference Poster
Abstract
The JWST Early Release Science Program 1386: “High Contrast Imaging of Exoplanets and Exoplanetary Systems includes a NIRISS aperture masking interferometry (AMI) component to demonstrate achievable contrast in a deep observation. As part of this program, we have developed SAMpy: data reduction tools tailored for NIRISS AMI, which are also flexible enough for arbitrary masking setups (e.g. LBT/LMIRCam, Keck/NIRC2, VLT/SPHERE). SAMpy takes a Fourier-plane approach to processing AMI data, which we describe here. We detail the individual pipeline steps, including image pre-processing, calculation and calibration of Fourier observables, OIFITS file generation, and model fitting. We also demonstrate SAMpy on NIRISS commissioning observations of the AB Dor system.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephanie Sallum, Shrishmoy Ray, and Sasha Hinkley "SAMpy: a Fourier-plane pipeline for JWST/NIRISS aperture masking interferometry (and more!)", Proc. SPIE 12183, Optical and Infrared Interferometry and Imaging VIII, 121832M (26 August 2022); https://doi.org/10.1117/12.2630401
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KEYWORDS
Calibration

James Webb Space Telescope

Visibility

Point spread functions

Interferometry

Stars

Data modeling

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